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Nov 25 at 18:52 comment added Asaf I would say it is more of "non stationary phase"/orthogonality. One clearly needs to integrate $d\mu$ (as the result is $t$ dependent). Now we see that when one fixes the $t$ value to the be value of Busemann cocycle (which will give you the length of the geodesic), it fixes $\mu$ also by orthogonality. The rest of $dzdb$ computation is basically verbatim as the regular computation of the orbital integral
Aug 6 at 2:58 comment added Dmitrii Korshunov >"the" prime geodesic< Since the surface is compact, every element of $\Gamma$ is hyperbolic. Also, any centralizer is a cyclic subgroup. From it it is easy to see in the upper half-plane model, after transforming the axis of the centralizer into a vertical line, that $F_\gamma$ is a domain between two concentric semi-circles and the prime geodesic is indeed unique [namely the part of the vertical line in the domain], any other geodesic segment will not glue up in the quotient.
Aug 4 at 5:43 history edited Daniele Tampieri CC BY-SA 4.0
Added some more detail to the reference paper
Aug 3 at 23:25 history asked Tsein32 CC BY-SA 4.0